Fig. 7.
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Best-fit star-forming MS shown at each redshift bin studied in this work as the solid black line. For comparison, we show the relations of Speagle et al. (2014), Tomczak et al. (2016) and Popesso et al. (2023), plotted with dashed blue, dash-dotted green, and dotted red lines, respectively. While all the functions tend to roughly agree with each other, some inconsistencies can clearly be seen, discussion of which is presented in Sect. 5.3.
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